{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:V35NPELEQA5FGT3KZGTHPPZW75","short_pith_number":"pith:V35NPELE","schema_version":"1.0","canonical_sha256":"aefad79164803a534f6ac9a677bf36ff566c543705ebd427b0bd139d1bc4163a","source":{"kind":"arxiv","id":"1605.05337","version":2},"attestation_state":"computed","paper":{"title":"Measurement of a Cosmographic Distance Ratio with Galaxy and CMB Lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alexander van Engelen, An\\v{z}e Slosar, Blake Sherwin, David N. Spergel, Hironao Miyatake, Mathew S. Madhavacheril, Neelima Sehgal","submitted_at":"2016-05-17T20:00:19Z","abstract_excerpt":"We measure the gravitational lensing shear signal around dark matter halos hosting CMASS galaxies using light sources at $z\\sim 1$ (background galaxies) and at the surface of last scattering at $z\\sim 1100$ (the cosmic microwave background). The galaxy shear measurement uses data from the CFHTLenS survey, and the microwave background shear measurement uses data from the {\\it Planck} satellite. The ratio of shears from these cross-correlations provides a purely geometric distance measurement across the longest possible cosmological lever arm. This is because the matter distribution around the h"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1605.05337","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2016-05-17T20:00:19Z","cross_cats_sorted":[],"title_canon_sha256":"62a7709e99eecb1b8b1e25a88820279e3a036e755b3a2a6dfac15f1cf8a9bca7","abstract_canon_sha256":"c6b3467c4f309d730fc9dce8ff9cbd20832f57d44369f406f246ce97b08512e8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:45:36.438696Z","signature_b64":"KOemH6NKlFc/EqJIYUbzj2LEO/7v8gYphfpcCYA66Nah//k4dCjXCqoGd+zYpPnvIGhTg0XL/JSaWp/SuWp8CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aefad79164803a534f6ac9a677bf36ff566c543705ebd427b0bd139d1bc4163a","last_reissued_at":"2026-05-18T00:45:36.437023Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:45:36.437023Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Measurement of a Cosmographic Distance Ratio with Galaxy and CMB Lensing","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Alexander van Engelen, An\\v{z}e Slosar, Blake Sherwin, David N. Spergel, Hironao Miyatake, Mathew S. Madhavacheril, Neelima Sehgal","submitted_at":"2016-05-17T20:00:19Z","abstract_excerpt":"We measure the gravitational lensing shear signal around dark matter halos hosting CMASS galaxies using light sources at $z\\sim 1$ (background galaxies) and at the surface of last scattering at $z\\sim 1100$ (the cosmic microwave background). The galaxy shear measurement uses data from the CFHTLenS survey, and the microwave background shear measurement uses data from the {\\it Planck} satellite. The ratio of shears from these cross-correlations provides a purely geometric distance measurement across the longest possible cosmological lever arm. This is because the matter distribution around the h"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.05337","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1605.05337","created_at":"2026-05-18T00:45:36.437221+00:00"},{"alias_kind":"arxiv_version","alias_value":"1605.05337v2","created_at":"2026-05-18T00:45:36.437221+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1605.05337","created_at":"2026-05-18T00:45:36.437221+00:00"},{"alias_kind":"pith_short_12","alias_value":"V35NPELEQA5F","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_16","alias_value":"V35NPELEQA5FGT3K","created_at":"2026-05-18T12:30:46.583412+00:00"},{"alias_kind":"pith_short_8","alias_value":"V35NPELE","created_at":"2026-05-18T12:30:46.583412+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75","json":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75.json","graph_json":"https://pith.science/api/pith-number/V35NPELEQA5FGT3KZGTHPPZW75/graph.json","events_json":"https://pith.science/api/pith-number/V35NPELEQA5FGT3KZGTHPPZW75/events.json","paper":"https://pith.science/paper/V35NPELE"},"agent_actions":{"view_html":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75","download_json":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75.json","view_paper":"https://pith.science/paper/V35NPELE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1605.05337&json=true","fetch_graph":"https://pith.science/api/pith-number/V35NPELEQA5FGT3KZGTHPPZW75/graph.json","fetch_events":"https://pith.science/api/pith-number/V35NPELEQA5FGT3KZGTHPPZW75/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75/action/storage_attestation","attest_author":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75/action/author_attestation","sign_citation":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75/action/citation_signature","submit_replication":"https://pith.science/pith/V35NPELEQA5FGT3KZGTHPPZW75/action/replication_record"}},"created_at":"2026-05-18T00:45:36.437221+00:00","updated_at":"2026-05-18T00:45:36.437221+00:00"}